Publications by authors named "Michele Ginolfi"

Article Synopsis
  • - Galaxy clusters are huge structures containing thousands of galaxies and a hot intracluster medium (ICM), which makes up much of their mass and changes over time due to matter accumulation and mergers with other clusters.
  • - Previous observations of the ICM have mostly focused on older clusters, leaving a gap in understanding the ICM during the formation of the first massive clusters.
  • - Recent detection of the thermal Sunyaev-Zeldovich effect in the Spiderweb protocluster shows the presence of a nascent ICM about 10 billion years ago, revealing a less intense signal than expected, indicating a younger, active cluster formation phase.
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